1 00:00:00,238 --> 00:00:02,695 - When we observe what we call fire 2 00:00:02,695 --> 00:00:04,707 we have this combustion reaction going on 3 00:00:04,707 --> 00:00:07,206 and then we see these flames 4 00:00:07,206 --> 00:00:08,628 what we're really observing 5 00:00:08,628 --> 00:00:12,571 are the three forms of thermal energy transfer. 6 00:00:12,571 --> 00:00:17,246 We're observing conduction, conduction, 7 00:00:17,246 --> 00:00:21,789 convection, convection, 8 00:00:21,789 --> 00:00:24,268 convection, 9 00:00:24,268 --> 00:00:27,968 and thermal radiation all at the same time. 10 00:00:27,968 --> 00:00:32,870 So I'll do this, thermal, thermal radiation, 11 00:00:32,870 --> 00:00:35,999 thermal radiation. 12 00:00:35,999 --> 00:00:37,218 And I could say thermal conduction, 13 00:00:37,218 --> 00:00:39,616 thermal convection, and thermal radiation, 14 00:00:39,616 --> 00:00:41,281 and the word thermal is just relating to things 15 00:00:41,281 --> 00:00:43,760 dealing with temperature. 16 00:00:43,760 --> 00:00:46,118 So what is the conduction going on? 17 00:00:46,118 --> 00:00:49,733 Well what we have going on in the fuel for our fire, 18 00:00:49,733 --> 00:00:52,375 so down here the fuel for our fire 19 00:00:52,375 --> 00:00:54,508 we have our classic combustion reaction 20 00:00:54,508 --> 00:00:56,174 and I encourage you to watch the video on that 21 00:00:56,174 --> 00:00:59,079 in our chemistry playlist, or chemistry section 22 00:00:59,079 --> 00:01:00,704 if you're interested in it. 23 00:01:00,704 --> 00:01:05,296 But you're taking carbon molecules and their bonds 24 00:01:05,296 --> 00:01:07,979 and then in the presence of oxygen and some heat 25 00:01:07,979 --> 00:01:09,726 you have a combustion reaction 26 00:01:09,726 --> 00:01:12,693 producing carbon dioxide and producing water 27 00:01:12,693 --> 00:01:15,617 and even more energy than you put into it, 28 00:01:15,617 --> 00:01:18,258 so it's producing a lot of energy. 29 00:01:18,258 --> 00:01:20,371 And that energy is going to excite 30 00:01:20,371 --> 00:01:21,673 the molecules that are around it, 31 00:01:21,673 --> 00:01:24,536 so you have these molecules, 32 00:01:24,536 --> 00:01:25,918 you have these molecules 33 00:01:25,918 --> 00:01:27,929 that end up getting a lot of kinetic energy. 34 00:01:27,929 --> 00:01:30,103 And remember, temperature is proportional 35 00:01:30,103 --> 00:01:32,094 to average kinetic energy. 36 00:01:32,094 --> 00:01:34,532 And so the ones that just combusted, 37 00:01:34,532 --> 00:01:36,767 or the molecules right near the reaction, 38 00:01:36,767 --> 00:01:38,636 or maybe the ones that were part of the reaction, 39 00:01:38,636 --> 00:01:39,998 they're gonna have this really high, 40 00:01:39,998 --> 00:01:43,614 they're gonna have this really high average kinetic energy 41 00:01:43,614 --> 00:01:45,382 'cause all of this energy was released 42 00:01:45,382 --> 00:01:47,455 from that combustion reaction. 43 00:01:47,455 --> 00:01:50,054 And then they're going to bump into other molecules 44 00:01:50,054 --> 00:01:53,244 that might not have quite as high kinetic energy, 45 00:01:53,244 --> 00:01:55,724 but then they're going to transfer that kinetic energy 46 00:01:55,724 --> 00:01:57,186 through these collisions. 47 00:01:57,186 --> 00:01:59,442 And we have a whole video on thermal conduction, 48 00:01:59,442 --> 00:02:00,559 but that's what's happening. 49 00:02:00,559 --> 00:02:01,900 Things with higher kinetic energy 50 00:02:01,900 --> 00:02:03,951 are bumping into things with lower kinetic energy 51 00:02:03,951 --> 00:02:06,025 and transferring some of that kinetic energy 52 00:02:06,025 --> 00:02:07,872 and they're transferring some of that momentum. 53 00:02:07,872 --> 00:02:09,538 So that is definitely happening 54 00:02:09,538 --> 00:02:12,058 when we look at a fire like this, 55 00:02:12,058 --> 00:02:13,969 that neighboring molecules are bumping 56 00:02:13,969 --> 00:02:16,996 into other molecules and transferring energy. 57 00:02:16,996 --> 00:02:19,617 Now convection, this is around the idea 58 00:02:19,617 --> 00:02:22,075 that hot air is less dense. 59 00:02:22,075 --> 00:02:25,305 So if we have a bunch of air particles here, 60 00:02:25,305 --> 00:02:28,333 so let's say this is the cool air up here, 61 00:02:28,333 --> 00:02:30,668 and it makes sense why cool air 62 00:02:30,668 --> 00:02:33,167 is going to be more dense than hot air. 63 00:02:33,167 --> 00:02:36,926 'Cause hot air, these particles have a much higher 64 00:02:36,926 --> 00:02:39,670 kinetic energy and so they're gonna bump 65 00:02:39,670 --> 00:02:41,498 into each other and they're gonna push each other 66 00:02:41,498 --> 00:02:45,743 much further away and get more seperation 67 00:02:45,743 --> 00:02:50,234 from each other because of that high average kinetic energy. 68 00:02:50,234 --> 00:02:53,952 But because the hot area is less dense, 69 00:02:53,952 --> 00:02:59,173 this area right over here is less dense, less dense, 70 00:02:59,173 --> 00:03:01,692 than the white area, these might be all the same molecule, 71 00:03:01,692 --> 00:03:03,136 I just made them in different colors to show 72 00:03:03,136 --> 00:03:05,147 the less dense area and the more dense area, 73 00:03:05,147 --> 00:03:07,950 it is going to rise, it is going to rise. 74 00:03:07,950 --> 00:03:08,945 Or you can even think of it 75 00:03:08,945 --> 00:03:10,775 as a more dense area. 76 00:03:10,775 --> 00:03:13,090 The more dense area is gonna fall around it, 77 00:03:13,090 --> 00:03:16,443 it's gonna fall around it, or try to go under it, 78 00:03:16,443 --> 00:03:17,784 because it is more dense, 79 00:03:17,784 --> 00:03:21,359 and then the less dense area is going to rise. 80 00:03:21,359 --> 00:03:22,436 And by doing that, 81 00:03:22,436 --> 00:03:27,415 you have the hotter molecules are moving upwards 82 00:03:27,415 --> 00:03:29,973 and then the cold molecules can go down 83 00:03:29,973 --> 00:03:33,285 to maybe the source of heat, the source of heat, 84 00:03:33,285 --> 00:03:35,196 the source of energy right over here 85 00:03:35,196 --> 00:03:36,577 to get heated up more. 86 00:03:36,577 --> 00:03:39,783 So this right over here is, so hot air rises, 87 00:03:39,783 --> 00:03:44,185 let me write this, the hot, hot air rises. 88 00:03:44,185 --> 00:03:44,930 And when we think about it 89 00:03:44,930 --> 00:03:47,148 it makes room for the cool air to come down 90 00:03:47,148 --> 00:03:48,505 and then get heated up again. 91 00:03:48,505 --> 00:03:50,334 And that's what's going on in the fire here. 92 00:03:50,334 --> 00:03:52,488 You see the combustion reaction, 93 00:03:52,488 --> 00:03:54,722 combustion reaction occurs right over there, 94 00:03:54,722 --> 00:03:56,104 let me just hit a different color, 95 00:03:56,104 --> 00:03:58,298 combustion reaction is occurring in the fuel, 96 00:03:58,298 --> 00:04:01,387 that super hot air, it's going to rise. 97 00:04:01,387 --> 00:04:02,810 And that's why it looks like these flames 98 00:04:02,810 --> 00:04:04,902 are kind of, they're moving upwards, 99 00:04:04,902 --> 00:04:06,893 they're kind of flickering upwards. 100 00:04:06,893 --> 00:04:08,498 And you'll also see, and actually we're gonna 101 00:04:08,498 --> 00:04:10,224 talk about this in thermal radiation, 102 00:04:10,224 --> 00:04:13,090 is that they also change color as they move upwards. 103 00:04:13,090 --> 00:04:16,016 But this whole idea of fire moving upwards 104 00:04:16,016 --> 00:04:17,274 and the hot air, 105 00:04:17,274 --> 00:04:19,326 if you put your hand up here it's gonna be much hotter 106 00:04:19,326 --> 00:04:24,263 than if you were to put your hand, say, right here, 107 00:04:24,263 --> 00:04:27,048 even though in theory this is closer to the flame 108 00:04:27,048 --> 00:04:30,075 than up here and that's because the hot air, 109 00:04:30,075 --> 00:04:33,101 the hot air is rising and it's making room for cold air, 110 00:04:33,101 --> 00:04:35,500 or cooler air, I guess I could say, 111 00:04:35,500 --> 00:04:37,511 to come down here and be part 112 00:04:37,511 --> 00:04:38,871 and get heated up again, 113 00:04:38,871 --> 00:04:40,762 and then it would rise up again. 114 00:04:40,762 --> 00:04:42,245 And so this convection, 115 00:04:42,245 --> 00:04:43,789 this idea of the hot air rising 116 00:04:43,789 --> 00:04:45,008 or the cold air falling, 117 00:04:45,008 --> 00:04:48,284 this is another form of heat transfer. 118 00:04:48,284 --> 00:04:50,255 Now the last form that we're observing 119 00:04:50,255 --> 00:04:53,303 when we're looking at fire is thermal radiation. 120 00:04:53,303 --> 00:04:55,193 And this is all around the idea 121 00:04:55,193 --> 00:04:58,585 that if you have charged particles being accelerated 122 00:04:58,585 --> 00:05:01,937 they're going to release electromagnetic radiation. 123 00:05:01,937 --> 00:05:03,746 And so you might say, Wait, wait, charged particles, 124 00:05:03,746 --> 00:05:05,899 where are those being accelerated here? 125 00:05:05,899 --> 00:05:07,260 Well, we have these molecules that are 126 00:05:07,260 --> 00:05:08,968 constantly being accelerated as they bump 127 00:05:08,968 --> 00:05:09,983 into each other, 128 00:05:09,983 --> 00:05:11,446 the one that's gonna transfer kinetic energy 129 00:05:11,446 --> 00:05:13,681 from, let's say this one bumps into that, 130 00:05:13,681 --> 00:05:15,225 it's going to accelerate that in different direction 131 00:05:15,225 --> 00:05:17,256 and even this one might go in another direction 132 00:05:17,256 --> 00:05:20,019 and acceleration is a change in velocity 133 00:05:20,019 --> 00:05:21,564 so it could be the magnitudinal velocity 134 00:05:21,564 --> 00:05:23,860 or your directional velocity. 135 00:05:23,860 --> 00:05:25,424 So as they're colliding you have all of these 136 00:05:25,424 --> 00:05:27,395 accelerational charged particles, 137 00:05:27,395 --> 00:05:28,817 so let me write this down, 138 00:05:28,817 --> 00:05:33,408 you have acceleration, acceleration 139 00:05:33,408 --> 00:05:38,737 of charged particles, charged particles, 140 00:05:39,036 --> 00:05:40,459 particles, 141 00:05:40,459 --> 00:05:44,075 and then that releases, that releases, 142 00:05:44,075 --> 00:05:46,187 electromagnetic radiation, 143 00:05:46,187 --> 00:05:48,869 that releases electromagnetic radiation. 144 00:05:48,869 --> 00:05:50,008 I know what you're thinking, Wait wait, 145 00:05:50,008 --> 00:05:51,165 hold on a second, Sal. 146 00:05:51,165 --> 00:05:54,173 Okay, I can buy that we have molecules 147 00:05:54,173 --> 00:05:55,452 that are being accelerated, 148 00:05:55,452 --> 00:05:57,260 but where is this charged, 149 00:05:57,260 --> 00:06:00,695 where are you getting this charged particles business? 150 00:06:00,695 --> 00:06:02,299 Well we have to remember these molecules 151 00:06:02,299 --> 00:06:04,514 are made up of atoms and atoms are made up of 152 00:06:04,514 --> 00:06:07,439 charged particles, are made up of protons and electrons. 153 00:06:07,439 --> 00:06:08,922 And so as you accelerate these 154 00:06:08,922 --> 00:06:10,182 and the more that you accelerate these 155 00:06:10,182 --> 00:06:13,860 the more radiation you are going to release. 156 00:06:13,860 --> 00:06:14,769 And you might say, Okay, 157 00:06:14,769 --> 00:06:16,405 you said I'm observing that in fire, 158 00:06:16,405 --> 00:06:18,372 where am I observing radiation? 159 00:06:18,372 --> 00:06:20,648 Well just the very fact that you can see the fire, 160 00:06:20,648 --> 00:06:22,639 the light emitted from the fire, 161 00:06:22,639 --> 00:06:25,626 that is electromagnetic radiation, 162 00:06:25,626 --> 00:06:27,840 that is electromagnetic radiation. 163 00:06:27,840 --> 00:06:29,242 It's just the electromagnetic radiation 164 00:06:29,242 --> 00:06:31,497 in the wavelengths that your eye 165 00:06:31,497 --> 00:06:32,980 considers to be visible light, 166 00:06:32,980 --> 00:06:34,910 or that your eye considers to be light. 167 00:06:34,910 --> 00:06:36,861 Even the particles up here, 168 00:06:36,861 --> 00:06:38,303 so even the particles up here 169 00:06:38,303 --> 00:06:39,665 that are still quite hot, 170 00:06:39,665 --> 00:06:43,078 they are also emitting electromagnetic radiation 171 00:06:43,078 --> 00:06:44,480 because they're all bumping into each other 172 00:06:44,480 --> 00:06:46,572 and their electrons and their protons 173 00:06:46,572 --> 00:06:49,031 are all getting accelerated in different ways, 174 00:06:49,031 --> 00:06:51,611 they're also releasing electromagnetic radiation, 175 00:06:51,611 --> 00:06:53,602 but it is at a slower wavelength 176 00:06:53,602 --> 00:06:57,056 than your eye is capable of perceiving as light. 177 00:06:57,056 --> 00:07:00,185 If you had an infrared camera 178 00:07:00,185 --> 00:07:02,663 you would see the flames being much larger. 179 00:07:02,663 --> 00:07:06,361 You would see them go all the way, all the way up here. 180 00:07:06,361 --> 00:07:08,982 And if you were to look at the flame closely 181 00:07:08,982 --> 00:07:11,339 you would see down here right where the 182 00:07:11,339 --> 00:07:13,472 combustion reaction is happening, 183 00:07:13,472 --> 00:07:15,280 the flame looks blue. 184 00:07:15,280 --> 00:07:17,149 And that's because the blue light 185 00:07:17,149 --> 00:07:18,409 is higher energy light, 186 00:07:18,409 --> 00:07:20,685 and that's because the particles are being accelerated 187 00:07:20,685 --> 00:07:21,721 more down here, 188 00:07:21,721 --> 00:07:24,951 and then it goes from blue to kind of a white 189 00:07:24,951 --> 00:07:28,568 to a yellow, to a red or to an orange, to a red, 190 00:07:28,568 --> 00:07:31,717 and then it, to your regular eyes, it disappears. 191 00:07:31,717 --> 00:07:34,094 But everything, everything that has some temperature 192 00:07:34,094 --> 00:07:36,715 is releasing electromagnetic radiation. 193 00:07:36,715 --> 00:07:38,726 And you're like, Okay, well that's all fine, 194 00:07:38,726 --> 00:07:41,510 I can see it but how is that a form of energy transfer? 195 00:07:41,510 --> 00:07:43,826 Well, if you're ever sat next to a flame 196 00:07:43,826 --> 00:07:45,309 you will feel the heat. 197 00:07:45,309 --> 00:07:48,397 In fact, even if the air between you and the flame is cold 198 00:07:48,397 --> 00:07:52,196 you would still feel like you're getting warm. 199 00:07:52,196 --> 00:07:55,447 So if this is a flame right over here, 200 00:07:55,447 --> 00:07:59,673 so that is fire, and let's say you have cold air, 201 00:07:59,673 --> 00:08:02,111 cold air, let's say you're at a campfire right over here, 202 00:08:02,111 --> 00:08:04,996 maybe it's 30, this air right over here is 30 degrees, 203 00:08:04,996 --> 00:08:09,161 if you are standing right over here 204 00:08:09,161 --> 00:08:11,172 you would still feel heat, 205 00:08:11,172 --> 00:08:13,306 you would still feel like you're getting warmed up. 206 00:08:13,306 --> 00:08:16,495 And that's because that electromagnetic radiation 207 00:08:16,495 --> 00:08:18,710 is being emitted from the air particles 208 00:08:18,710 --> 00:08:21,168 that we perceive as fire 209 00:08:21,168 --> 00:08:23,220 and then that can actually excite particles 210 00:08:23,220 --> 00:08:24,500 on your skin 211 00:08:24,500 --> 00:08:26,999 and it will transfer energy to your skin 212 00:08:26,999 --> 00:08:30,981 and so you feel like you are actually getting warmed up. 213 00:08:30,981 --> 00:08:33,501 I remember once, this is kind of a strange story, 214 00:08:33,501 --> 00:08:35,472 but I was on the highway 215 00:08:35,472 --> 00:08:36,832 and there was a car on fire 216 00:08:36,832 --> 00:08:39,758 and I was literally, we drove to the far lane 217 00:08:39,758 --> 00:08:40,774 because it was on fire, 218 00:08:40,774 --> 00:08:42,054 we're three lanes away from it 219 00:08:42,054 --> 00:08:43,517 and it kind of exploded. 220 00:08:43,517 --> 00:08:45,163 I don't think anyone was in it, 221 00:08:45,163 --> 00:08:46,280 hopefully no one was in it, 222 00:08:46,280 --> 00:08:47,702 but I remember right when it exploded 223 00:08:47,702 --> 00:08:50,851 it was an intense, immediate heat that we felt 224 00:08:50,851 --> 00:08:52,517 through the window of the car, 225 00:08:52,517 --> 00:08:55,565 and that was electromagnetic radiation. 226 00:08:55,565 --> 00:08:57,312 That was thermal radiation being released 227 00:08:57,312 --> 00:08:58,999 by these accelerated particles 228 00:08:58,999 --> 00:09:01,335 in the air around that explosion, 229 00:09:01,335 --> 00:09:04,118 which we perceived as a an explosion, or fire, 230 00:09:04,118 --> 00:00:00,000 but then it was warming up particles on my skin.